Temperature
This section aims to elucidate the concepts of temperature in relation to solar radiation and the heat balance of the Earth. The interaction between incoming solar radiation, termed insolation, and the atmosphere is critical in determining temperature variations across different regions.
The Earth primarily receives energy from the sun, which it radiates back into space, maintaining a balance that prevents it from warming excessively or cooling down. Insolation varies due to factors including the Earth's axial tilt and its distance from the sun, affecting temperatures globally. The section elaborates on the distribution of energy received across different latitudes, highlighting the greater heating in the tropics versus the poles.
Furthermore, it discusses the heating mechanisms in the atmosphere, namely conduction, convection, and advection, explaining how heat is transferred within atmospheric layers. The heat budget concept is introduced, showcasing how absorbed and radiated energy achieves equilibrium overall, while individual factors, such as latitude, altitude, and proximity to water bodies, determine local temperature distributions. Inversion of temperature is also covered, illustrating anomalies in standard temperature decrease with increased elevation.